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dc.contributor.authorGoodger, Joanna
dc.contributor.authorHardcastle, M.J.
dc.contributor.authorCroston, J.H.
dc.date.accessioned2008-06-27T14:12:24Z
dc.date.available2008-06-27T14:12:24Z
dc.date.issued2008
dc.identifier.citationGoodger , J , Hardcastle , M J & Croston , J H 2008 , Inverse-Compton Emission from the Lobes of 3C353 . in Extragalactic Jets: Theory and Observation from Radio to Gamma Ray . ASP Conf Series , vol. 386 , Astronomical Society of the Pacific , pp. 363-365 .
dc.identifier.isbn978-1-58381-336-2
dc.identifier.isbn978-1-58381-335-5
dc.identifier.otherPURE: 160812
dc.identifier.otherPURE UUID: 775c9e6e-002d-4f6a-9795-f666225f7d88
dc.identifier.otherdspace: 2299/2135
dc.identifier.urihttp://hdl.handle.net/2299/2135
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/381.html Copyright ASP
dc.description.abstractAnalysis of the radio synchrotron and X-ray inverse-Compton emission from radio-loud active galaxies allows us to determine their particle ac- celeration processes and electron energy spectra. Previous studies have provided new constraints on the total energy budget and particle content of powerful radio galaxies and quasars; however, in most cases the sources are too faint in the X-ray to obtain spatial information. We present archival and new multi-frequency radio observations from the VLA and GMRT, and XMM-Newton observations of the bright FRII radio galaxy 3C353 which lies on the edge of the X-ray-luminous cluster Zw 1718.1-0108. The X-ray observations detect both the inverse-Compton emission from the radio galaxy lobes and thermal emission from the hot phase of the intracluster medium. We discuss the properties of the particle energy spectrum as a function of position in the lobe, as well as the properties of the merging cluster.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofExtragalactic Jets: Theory and Observation from Radio to Gamma Ray
dc.relation.ispartofseriesASP Conf Series
dc.titleInverse-Compton Emission from the Lobes of 3C353en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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